-
Massive stars in nearby galaxies
Mass loss is a key aspect of stellar evolution, particularly in evolved massive stars, yet episodic mass loss remains poorly understood. To investigate this, we need evolved... -
9Msun ultramassive WD stars progenitor
We study the full evolution of a 1.313M_{sun} white dwarf star that descended from a 9M{sun} main-sequence progenitor with an initial metallicity of Z=0.02. Using MESA... -
Ultraviolet spectroscopy of MWC 656
The Galactic Be star binary MWC 656 was long considered the only known Be star +black hole (BH) system, making it a critical benchmark for models of massive binary evolution and... -
Single-lined spectroscopic orbits RVs
Massive stars play crucial roles in galactic dynamics and chemical evolution. They are the most significant sources of ionizing UV radiation, their substantial mass-loss rates... -
Massive stars in the Milky Way
Massive stars play a significant role in different branches of astronomy, from shaping the processes of star and planet formation to influencing the evolution and chemical... -
Kinematic data for O-B5 stars
This document describes the magnetic tape version of a catalog of 1440 O-B5 star with radial velocities accurate to within 5 km/sec, located within 3 kpc of the sun and within... -
Parameters for the 172 {lambda} Boo stars
The evolutionary status of the chemically peculiar class of {lambda} Boo stars has been intensely debated. It is now agreed that the {lambda} Boo phenomenon affects A stars of... -
Deep OB star population in Carina
Massive OB stars are critical to the ecology of galaxies, and yet our knowledge of OB stars in the Milky Way, fainter than V~12, remains patchy. Data from the VST Photometric... -
New hot subdwarf stars
Recent massive sky surveys in different bandwidths are providing new opportunities to modern astronomy. The Virtual Observatory (VO) represents the adequate framework to handle... -
Young clumps embedded in IRDC
We present a catalogue of starless and protostellar clumps associated with infrared dark clouds (IRDCs) in a 40 degrees wide region of the inner Galactic plane (|b|<=1). We... -
Extended H2 emission from massive YSOs survey
We present the results from a survey, designed to investigate the accretion process of massive young stellar objects (MYSOs) through near infrared narrow band imaging using the... -
Intermediate high-velocity clouds distances
We present optical spectra of 403 stars and quasi-stellar objects in order to obtain distance limits towards intermediate- and high-velocity clouds (IHVCs), including new... -
Fitted UBV magnitude for MS stars
We fit the colour-magnitude diagrams of stars between the zero-age main-sequence and terminal-age main sequence in young clusters and associations. The ages we derive are a... -
Lower main-sequence stars fundamental param.
We derive an empirical effective temperature and bolometric luminosity calibration for G and K dwarfs, by applying our own implementation of the Infrared Flux Method to... -
Metallicity calibrations for UBV photometry
Calibrations are presented here for metallicity ([Fe/H]) in terms of the ultraviolet excess, [{Delta}(U-B) at B-V=0.6, hereafter D0.6], and also for the absolute visual... -
Interstellar NaI, TiII & CaIIK obs.
We present an analysis of interstellar NaI ({lambda}air=3302.37 and 3302.98{AA}), TiII ({lambda}air=3383.76{AA}) and CaIIK ({lambda}air=3933.66{AA}) absorption features for 74... -
2dF survey of the Small Magellanic Cloud
We present a catalogue of new spectral types for hot, luminous stars in the Small Magellanic Cloud. The catalogue contains 4161 objects, giving an order of magnitude increase in... -
Circumstellar Disks of Ae/Be Herbig Stars
The data of the photo-polarimetric activity of Ae/Be Herbig stars and the types of Ha profiles observed in their spectra was carried out using data from the literature. The... -
Synthetic UV spectra of massive stars
An atlas of synthetic ultraviolet spectra of a population of massive stars is presented. The spectra are based on a stellar library of IUE high-dispersion spectra of O and... -
Far UV Stellar Photometry
Far-ultraviolet photometry for 741 objects in a field in Sagittarius centered near M8 and 541 objects in a field centered near zeta Scorpii is presented. These data were...
